Neutron-Driven Nucleosynthesis in Stellar Plasma

Neutron-Driven Nucleosynthesis in Stellar Plasma

A large uncertainty for the slow neutron capture nucleosynthesis (s-process) models is caused by the amount of neutrons available to the process itself. This quantity is strongly affected by the 13C(α,n)16O, and 22Ne(α,n)25Mg reaction cross sections, whose measurements at energies corresponding to t...

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Bibliographic Details
Main Authors: R. Spartà, M. La Cognata, G. L. Guardo, S. Palmerini, M. L. Sergi, G. D’Agata, L. Lamia, D. Lattuada, A. A. Oliva, R. G. Pizzone, G. G. Rapisarda, S. Romano, A. Tumino
Format: Article
Language:English
Published: Frontiers Media S.A. 2022-05-01
Series:Frontiers in Physics
Subjects:
neutron induced reactions
stellar evolution
nucleosynthesis
indirect process
s-process
Online Access:https://www.frontiersin.org/articles/10.3389/fphy.2022.896011/full

Internet

https://www.frontiersin.org/articles/10.3389/fphy.2022.896011/full

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